PL EN


Preferencje help
Widoczny [Schowaj] Abstrakt
Liczba wyników
Czasopismo
2015 | 13 | 1 |
Tytuł artykułu

Kantowski-Sachs Cosmological model with quark and strange quark matter inf(R) theory of gravity

Treść / Zawartość
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
In this paper we have studied the Kantowski- Sachs cosmological model with the quark and strange quark matter in the f (R) theory of gravity. The general solutions of the field equations are obtained by assuming the physical condition shear scalar σ is proportional to scalar expansion θ, which leads to the relation B = An between metric coefficients B and A. The physical and geometrical aspects of the model are also discussed.
Wydawca

Czasopismo
Rocznik
Tom
13
Numer
1
Opis fizyczny
Daty
wydano
2015-01-01
otrzymano
2014-06-08
zaakceptowano
2014-09-15
online
2014-11-03
Twórcy
  • Department of Mathematics, Sant Gadge Baba
    Amravati University, Amravati 444602, India
  • Department of Mathematics, Sant Gadge Baba
    Amravati University, Amravati 444602, India
Bibliografia
  • [1] A.G. Riess et al., Astron. J. 116, 1009 (1998)
  • [2] S. Perlmutter et al., Astrophys. J. 517, 565 (1999)
  • [3] P. de Bernardis et al., Nature 404, 955 (2000)
  • [4] S. Hanany et al., Astrophys. J. 545, L5 (2000)
  • [5] P.J.E. Peebles, B. Ratra, Rev. Mod. Phys. 75, 559 (2003)
  • [6] T. Padmanabhan, Phys. Rept. 380, 235 (2003)
  • [7] S.M. Carroll et al., Phys. Rev. D 70, 043528 (2004)
  • [8] S. Capozziello, V. Faraoni, Beyond Einstein Gravity (Springer,New York, 2010)
  • [9] A. Elizalde et al., Phys. Rev. D 83, 086006 (2011)
  • [10] M.K. Mak, T. Harko, Int. J. Mod. Phys. D 13, 149 (2004)[Crossref]
  • [11] I. Yavuz et al., Int. J. Mod. Phys. D 14, 1365 (2005)[Crossref]
  • [12] K.S. Adhav et al., Int. J. Theor. Phys. 47, 2002 (2008)
  • [13] K.S. Adhav et al., Astrophys. Space Sci. 319, 81 (2009)
  • [14] S.D. Katore, Int. J. Theor. Phys. 51, 83 (2012)
  • [15] I. Yilmaz et al., Gen. Relat. Gravit. 44, 2313 (2012)
  • [16] K.S. Adhav, Can. J. Phys. 90, 119 (2012)
  • [17] P.K. Sahoo, B. Mishra, IJPAM 82, 87 (2013)
  • [18] R. Kantowaski, R.K. Sachs, J. Math. Phys. 7, 433 (1966)
  • [19] M. Sharif, M.F. Shamir, Class. QuantumGrav. 26, 235020 (2009)[Crossref]
  • [20] M. Sharif, M.F. Shamir, Gen. Relat. Grav. 42, 2643 (2010)[Crossref]
  • [21] J. Adams et al. (STAR Collaboration), Nucl. Phys. A 757, 102(2005)
  • [22] K. Adcox et al. (PHENIX Collaboration), Nucl. Phys. A 757, 184(2005)
  • [23] B.B. Back et al. (PHOBOS Collaboration), Nucl. Phys. A 757, 28(2005)
  • [24] C. Aktas et al., Gen. Relat. Gravit. 43, 1577 (2011)[Crossref]
  • [25] R. Sharma et al., IJMPD 15, 405 (2006)
  • [26] R. Sharma et al., MNRAS, 375, 1265 (2007)
  • [27] J. Kristian, R.K. Sachs, Astrophys. J. 143, 379 (1966)
  • [28] K.S. Thorne, Astrophys. J. 148, 51 (1967)
  • [29] C.B. Collins, E.N. Glass, D.A. Wilkinson, Gen. Relat. Gravit. 12,805 (1980)[Crossref]
  • [30] A.K. Banerjee, N.O. Santos, Gen. Relat. Gravit. 16, 217 (1984)[Crossref]
  • [31] X.X. Wang, Chin. Phys. Lett. 22, 29 (2005)[Crossref]
  • [32] A. Pradhan, Fizika B 16, 205 (2007)
  • [33] A. Pradhan, A.K. Yadav, R.R. Singh, V.K. Singh, Astrophys. SpaceSci. 312, 3 (2007)
  • [34] A. Pradhan, A.K. Jotani, A. Singh, Braz. J. Phys. 38, 167 (2008)[Crossref]
  • [35] M.F. Shamir, Gen. Relat. Grav. 42, 1557 (2010)
  • [36] R. Venkateswarlu, J. Satish, K. Pavan Kumar, Elect. J. Theor.Phys. 8, 353 (2011)
  • [37] M. Sharif, S. Waheed, Eur. Phys. J. C 72, 1876 (2012)
  • [38] D.R.K. Reddy, Ch. Purnachandra Rao, T. Vidyasagar, R. Bhuvana,Adv. High Energy Phys. 2013, 609807 (2013)
  • [39] V.B. Johri, K. Desikan, Gen. Relat. Grav. 26, 1217 (1994)[Crossref]
  • [40] K. Uddin et al., Class. Quantum Grav. 24, 3951 (2007)[Crossref]
  • [41] S. Perlmutter et al., Nature (London) 319, 51 (1998)
  • [42] R.K. Knop et al., Astrophys. J. 598, 102 (2003)
Typ dokumentu
Bibliografia
Identyfikatory
Identyfikator YADDA
bwmeta1.element.-psjd-doi-10_1515_phys-2015-0010
JavaScript jest wyłączony w Twojej przeglądarce internetowej. Włącz go, a następnie odśwież stronę, aby móc w pełni z niej korzystać.